Formation and evolution of dust in novae

Details Formation and evolution of dust in novae Formation and evolution of dust in novae

Nov 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aipc..637..270r&link_type=abstract

CLASSICAL NOVA EXPLOSIONS: International Conference on Classical Nova Explosions. AIP Conference Proceedings, Volume 637, pp. 2

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3

Novae, Dwarf Novae, Recurrent Novae, And Other Cataclysmic Variables

Scientific paper

We discuss the formation and evolution dust in nova winds. The ability of a nova to produce carbon and/or silicate dust is determined by the propagation of ionization fronts through the ejected material rather than by a single nova parameter (such as speed class). We also describe the changing physical and chemical properties of the dust as the stellar and gaseous remnants evolve.

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